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Black hole and cosmological space-times in Born-Infeld-Einstein theory

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arxiv gr-qc/0601136 v1 pith:25PNXXE7 submitted 2006-01-30 gr-qc

classification gr-qc
keywords space-timesblackborn-infeldcosmologicalsingularitysphericallysymmetrictheory
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abstract

In this paper I examine black hole and cosmological space-times in Born-Infeld-Einstein theory with electric and magnetic charges. The field equations are derived and written in the form $G_{\mu\nu}=-\kappa T_{\mu\nu}$ for spherically symmetric space-times. The energy-momentum tensor is not the Born-Infeld energy-momentum tensor, but can be obtained from Born-Infeld theory by letting $a\to ia$, where $a$ is the Born-Infeld parameter. It is shown that there is a curvature singularity in spherically symmetric space-times at a nonzero radial coordinate and that, as in Reissner-Nordstrom space-times, there are zero, one or two horizons. Charged black holes have either two horizons and a timelike singularity or one horizon with a spacelike, timelike, or null singularity. Anisotropic cosmological solutions with electric and magnetic fields are obtained from the spherically symmetric solutions.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Born-Infeld Electrogravity and Dyonic Black Holes

    gr-qc 2025-11 unverdicted novelty 6.0 of 10

    Born-Infeld electrogravity yields a fundamental extremal dyonic black hole in the small-charge limit whose mass and horizon area depend only on the Born-Infeld constant, Newton’s constant, and the speed of light.

  2. Eddington-inspired Born-Infeld gravity: Constraints from the generalized parton distributions (GPDs)

    hep-ph 2025-05 reject novelty 4.0 of 10

    Using the proton's quark pressure profile from a GPD fit, the authors update upper bounds on the EiBI gravity parameter kappa to about 0.1 to 0.3 in the quoted units.

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